Viable cosmology in bimetric theory

被引:87
|
作者
De Felice, Antonio [1 ]
Guemruekcueoglu, A. Emir [2 ,3 ]
Mukohyama, Shinji [3 ]
Tanahashi, Norihiro [3 ,4 ]
Tanaka, Takahiro [1 ,5 ]
机构
[1] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
[2] Univ Nottingham, Sch Math Sci, Nottingham NG7 2RD, England
[3] Univ Tokyo, Kavli Inst Phys & Math Universe, Todai Inst Adv Study, WPI, Kashiwa, Chiba 2778583, Japan
[4] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA, England
[5] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan
基金
欧洲研究理事会;
关键词
modified gravity; cosmological perturbation theory; MASSIVE GRAVITY; RANGE;
D O I
10.1088/1475-7516/2014/06/037
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study cosmological perturbations in bimetric theory with two fluids each of which is coupled to one of the two metrics. Focusing on a healthy branch of background solutions, we clarify the stability of the cosmological perturbations. For this purpose, we extend the condition for the absence of the so-called Higuchi ghost, and show that the condition is guaranteed to be satisfied on the healthy branch. We also calculate the squared propagation speeds of perturbations and derive the conditions for the absence of the gradient instability. To avoid the gradient instability, we find that the model parameters are weakly constrained.
引用
收藏
页数:22
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